Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Cancer |
Right ascension | 08h01m 30.28830s[1] |
Declination | +16° 27′ 19.1191″[1] |
Apparent magnitude (V) | 5.99[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | B9.5 Vn[4] |
B−V color index | −0.024±0.003[2] |
Astrometry | |
Radial velocity (Rv) | −10.0±1.5[5] km/s |
Proper motion (μ) | RA: +4.12[6] mas/yr Dec.: −5.43[6] mas/yr |
Parallax (π) | 6.2251 ± 0.1419 mas[1] |
Distance | 520 ± 10 ly (161 ± 4 pc) |
Absolute magnitude (MV) | −0.09[2] |
Details | |
Mass | 2.93±0.10[3] M☉ |
Radius | 3.1[7] R☉ |
Luminosity | 121.1+20.2 −17.3[3] L☉ |
Surface gravity (log g) | 4.5[4] cgs |
Temperature | 9,727+90 −89[3] K |
Rotational velocity (v sin i) | 188[3] km/s |
Age | 36[4] Myr |
Other designations | |
5 Cnc, BD+16°1612, HD 65873, HIP 39236, HR 3134, SAO 97485[8] | |
Database references | |
SIMBAD | data |
5 Cancri is a single[9] star in the zodiac constellationofCancer, located around 520 light years away from the Sun. It is just visible to the naked eye under good seeing conditions as a dim, blue-white hued star with an apparent visual magnitude of 5.99.[2] This object is moving closer to the Sun with a heliocentric radial velocity of −10 km/s.[5]
At one point this was thought to be a spectroscopic binary system. It is a Be star with a weak circumstellar disk of gas that has around three times the radius of the host star.[10] The stellar classification of 5 Cancri is B9.5 Vn,[4] matching a B-type main-sequence star with "nebulous" lines due to rapid rotation. It is 36[4] million years old with a high projected rotational velocity of 188 km/s.[3] The star has 2.9[3] times the mass of the Sun and about 3.1[7] times the Sun's radius. It is radiating 121[3] times the Sun's luminosity from its photosphere at an effective temperature of 9,727 K.[3]
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